2MASX J08021869+3046228 , the SIMBAD biblio

2MASX J08021869+3046228 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST19:56:25


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Title First 3 Authors
2003A&A...412...45P viz 15       D               1 956189 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
2008AJ....136.2373R viz 890 251 Space density of optically selected type 2 quasars. REYES R., ZAKAMSKA N.L., STRAUSS M.A., et al.
2009MNRAS.393.1408C viz 504 3 Infrared photometric study of type II quasars. CHEN P.S. and SHAN H.G.
2009ApJ...705L..76W viz 90       D       C       2 93 141 Active galactic nuclei with double-peaked narrow lines: are they dual active galactic nuclei? WANG J.-M., CHEN Y.-M., HU C., et al.
2010ApJ...708..427L viz 15       D               1 174 147 Type 2 active galactic nuclei with double-peaked [O III] lines: narrow-line region kinematics or merging supermassive black hole pairs? LIU X., SHEN Y., STRAUSS M.A., et al.
2010A&A...518A..10V viz 15       D               1 168913 597 A catalogue of quasars and active nuclei: 13th edition. VERON-CETTY M.-P. and VERON P.
2012MNRAS.421.1043S viz 15       D               2 3198 151 Strongly star forming galaxies in the local Universe with nebular He II λ4686 emission. SHIRAZI M. and BRINCHMANN J.
2012ApJ...753...42C viz 15       D               1 82 81 Kiloparsec-scale spatial offsets in double-peaked narrow-line active galactic nuclei. I. Markers for selection of compelling dual active galactic nucleus candidates. COMERFORD J.M., GERKE B.F., STERN D., et al.
2012ApJS..201...31G viz 15       D               1 15563 75 Double-peaked narrow emission-line galaxies from the Sloan Digital Sky Survey. I. Sample and basic properties. GE J.-Q., HU C., WANG J.-M., et al.
2014ApJ...788...45T viz 15       D               1 224166 54 Luminosity and redshift dependence of the covering factor of active galactic nuclei viewed with WISE and Sloan Digital Sky Survey. TOBA Y., OYABU S., MATSUHARA H., et al.
2015ApJ...813..103M 290       D     X C       7 43 98 The origin of double-peaked narrow lines in active galactic nuclei. I. Very large array detections of dual AGNs and AGN outflows. MULLER-SANCHEZ F., COMERFORD J.M., NEVIN R., et al.
2016ApJ...832...67N viz 94       D       C       3 71 19 The origin of double-peaked narrow lines in active galactic nuclei. II. Kinematic classifications for the population at z < 0.1. NEVIN R., COMERFORD J., MULLER-SANCHEZ F., et al.
2018ApJ...859..116K viz 16       D               1 888 24 The black hole masses and Eddington ratios of type 2 quasars. KONG M. and HO L.C.
2019MNRAS.484.4933R 16       D               1 88 28 Searching for dual AGN in galaxies with double-peaked emission line spectra using radio observations. RUBINUR K., DAS M. and KHARB P.
2019ApJ...873...90S 16       D               1 87 4 Testing the evolutionary link between type 1 and type 2 quasars with measurements of the interstellar medium. SHANGGUAN J. and HO L.C.
2020ApJS..247...53K viz 16       D               1 23378 20 Radio sources associated with Optical Galaxies and having Unresolved or Extended morphologies (ROGUE). I. A catalog of SDSS galaxies with FIRST core identifications. KOZIEL-WIERZBOWSKA D., GOYAL A. and ZYWUCKA N.
2022MNRAS.509.3966W viz 17       D               1 89291 61 Galaxy Zoo DECaLS: Detailed visual morphology measurements from volunteers and deep learning for 314 000 galaxies. WALMSLEY M., LINTOTT C., GERON T., et al.
2022MNRAS.512...86B viz 17       D               1 304 3 Quantifying the cool ISM in radio AGNs: evidence for late-time retriggering by galaxy mergers and interactions. BERNHARD E., TADHUNTER C.N., PIERCE J.C.S., et al.
2023MNRAS.518..130S viz 104       D       C       3 813 1 Efficient analysis routines for single and double peaked Type 2 AGN spectra. SELWOOD M., CALDERONE G., FOTOPOULOU S., et al.
2025ApJ...981..194L 19       D               5 182 ~ Measuring the Interstellar Medium Content of Nearby, Luminous, Type 1 and Type 2 QSOs through CO and [C II]. LUO Y., PETRIC A.O., JANSSEN R.M.J., et al.

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